We present a detailed examination of the variational principle for metric general relativity as applied to a quasilocal spacetime region M (that is, a region that is both spatially and temporally bounded). Our analysis relies on the Hamiltonian formulation of general relativity and thereby assumes a
The Gravitational Field of Deimos
β Scribed by David Parry Rubincam; Benjamin Fong Chao; Peter C. Thomas
- Publisher
- Elsevier Science
- Year
- 1995
- Tongue
- English
- Weight
- 251 KB
- Volume
- 114
- Category
- Article
- ISSN
- 0019-1035
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β¦ Synopsis
Deimos may be largely uniform in density. We find here the gravitational field of Deimos and its moments of inertia from the moon's shape and an assumed uniform density distribution. From these data we compute the expected orientation. The orientation of the model Deimos relative to Mars agrees with that observed to within the observation uncertainties (a few degrees). Hence Deimos may be homogeneous and not have significant density variations in its interior. We also find that the spherical harmonic coefficient (J_{2}) is about 0.108 for the model, so that Deimos is about as gravitationally flattened as Phobos, whose (J_{2}) is about 0.105. 1995 Academic Press, Inc.
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